File:15 fe eqwidth.gif
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How the equivalent width of the Fe feature compares with theory for many points during a particular solar flare. Basically the flare evolution moves the points up in temperature rapidly, then more slowly downwards. At this level, the discrepancy is probably not significant yet.
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 01:24, 23 January 2010 |  | 800×677 (48 KB) | Schriste (Talk | contribs) | (How the equivalent width of the Fe feature compares with theory for many points during a particular solar flare. Basically the flare evolution moves the points up in temperature rapidly, then more slowly downwards. At this level, the discrepancy is probab) |
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